Interplanetary Meteoroids Near Earh and Moon

Details Interplanetary Meteoroids Near Earh and Moon Interplanetary Meteoroids Near Earh and Moon

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008epsc.conf..717d&link_type=abstract

European Planetary Science Congress 2008, Proceedings of the conference held 21-25 September, 2008 in Münster, Germany. Online a

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Several models for the sporadicmeteoroid background have been developed over the last two decades. These include, among others, the Divine, the Staubach and the Dikarev model. They cover mass ranges from 10-18 g to 1 g typically and are applicable for model-specific heliocentric distance ranges between 0.1 and 20 AU. At 1 AU from the Sun in the ecliptic plane, averaged fluxes (over directions and velocities) are tuned to the well established interplanetary model by Grün et al. (1985). However, in many respects thesemodels differ considerably, and our comparison of flux predictions near Earth from existing models shows a clear need for additional measurements and simulations in order to derive a reliable model for the population of interplanetary and interstellar meteoroids.

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